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Solar 3D models vs. observations - a few comments
Stockholm University, Faculty of Science, Department of Astronomy. KVA:s institut för solfysik.
2008 (English)In: Physica Scripta, Vol. T133, 014016- p.Article in journal (Other academic) Published
Abstract [en]

Some properties of 3D solar photospheric models and the observations used to test them are

discussed: granulation contrast and spectral line variation in the granulation pattern and over

the solar disc. The recent use of the techniques of solar physics to tackle abundance problems

is encouraged.

Place, publisher, year, edition, pages
2008. Vol. T133, 014016- p.
National Category
Astronomy, Astrophysics and Cosmology
URN: urn:nbn:se:su:diva-18416OAI: diva2:184939
Available from: 2009-01-26 Created: 2009-01-26 Last updated: 2011-01-10Bibliographically approved

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Kiselman, Dan
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